Pure dephasing in flux qubits due to flux noise with spectral density scaling as $1/ f^\alpha$
S. M. Anton, C. M\"uller, J. S. Birenbaum, S. R. O'Kelley, A. D., Fefferman, D. S. Golubev, G. C. Hilton, H.-M. Cho, K. D. Irwin, F. C., Wellstood, Gerd Sch\"on, A. Shnirman, and John Clarke

TL;DR
This paper investigates how flux noise with a $1/f^eta$ spectral density affects the pure dephasing times of superconducting flux qubits, revealing that the spectral exponent significantly influences qubit coherence.
Contribution
It provides a detailed analysis of the impact of flux noise spectral scaling on qubit dephasing, including the dependence on the spectral exponent and the cutoff frequencies, which was not previously characterized.
Findings
Dephasing time decreases rapidly as the spectral exponent $eta$ decreases.
Dephasing times are relatively insensitive to the noise bandwidth if the ultraviolet cutoff exceeds $1/\tau_\phi$.
The choice of pivot frequency $f_0$ significantly affects the sensitivity of dephasing times to the spectral exponent.
Abstract
For many types of superconducting qubits, magnetic flux noise is a source of pure dephasing. Measurements on a representative dc superconducting quantum interference device (SQUID) over a range of temperatures show that , where is the flux noise spectral density, is of the order of 1 and ; is the flux quantum. For a qubit with an energy level splitting linearly coupled to the applied flux, calculations of the dependence of the pure dephasing time of Ramsey and echo pulse sequences on for fixed show that decreases rapidly as is reduced. We find that is relatively insensitive to the noise bandwidth, , for all provided the ultraviolet cutoff frequency . We…
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Taxonomy
TopicsAtomic and Subatomic Physics Research
